ARCHIVE RATAN-600 Observation Schedule
from 1 July to 31 December, 2019


Executive Secretary: request@sao.ru
Russian version

  North Sector South+Flat South Sector West Sector
J
U
L
Y

Feed-cabin 1

(01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Mikhailov A.G.

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-31): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

Feed-cabin 3

(01-31): The Sun five-azimuth observations 3.
Responsible Kazanina T.N.

(01-31): Repairs,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-31): Antenna measurements,
AMG (SAO RAS).
Responsible Zharov V.I.

(01-31): Repairs,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-31): Antenna measurements,
AMG (SAO RAS).
Responsible Zharov V.I.

Feed-cabin 5

(01-31): Test observations (SAO RAS).
Responsible Trushkin S.A.

A
U
G
U
S
T

Feed-cabin 1

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-10): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees,
Konnikova V.K. (SAI MSU).
Responsible Erkenov A.K.

(11-31): Radio properties of the distant quasars,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(11-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Mikhailov A.G.

Feed-cabin 3

(01-31): The Sun five-azimuth observations 3.
Responsible Kazanina T.N.

(01-31): Repairs,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-31): Antenna measurements,
AMG (SAO RAS).
Responsible Zharov V.I.

(01-31): Repairs,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-31): Antenna measurements,
AMG (SAO RAS).
Responsible Zharov V.I.

Feed-cabin 5

(01-31): Test observations (SAO RAS).
Responsible Trushkin S.A.

S
E
P
T
E
M
B
E
R

Feed-cabin 1

(01-30): The AGN study with the RATAN-600 and VLBI 2,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

(01-30): Radio variability of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 3

(01-30): The Sun five-azimuth observations 3.
Responsible Kazanina T.N.

(01-30): Repairs,
MS R-600 (SAO RAS)

(01-30): Antenna measurements,
AMG (SAO RAS).
Responsible Zharov V.I.

(01-30): Repairs,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-30): Antenna measurements,
AMG (SAO RAS).
Responsible Zharov V.I.

Feed-cabin 5

(01-30): Test observations (SAO RAS).
Responsible Trushkin S.A.

O
C
T
O
B
E
R

Feed-cabin 1

(01-01): The AGN study with the RATAN-600 and VLBI 2,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

(01-01): Radio variability of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(02-04): Reserve time (SAO RAS)

(05-17): Technical support,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(18-31): Adjustment, antenna measurements,
AMG, RAL (SAO RAS).
Responsible Zharov V.I., Trushkin S.

Feed-cabin 3

(01-31): The Sun five-azimuth observations 3.
Responsible Kazanina T.N.

(01-31): Repairs,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-31): Antenna measurements,
AMG (SAO RAS).
Responsible Zharov V.I.

(01-31): Repairs,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-31): Antenna measurements,
AMG (SAO RAS).
Responsible Zharov V.I.

Feed-cabin 5

(01-31): Test observations (SAO RAS).
Responsible Trushkin S.A.

N
O
V
E
M
B
E
R

Feed-cabin 1

(01-02): Reserve time

(03-30): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(03-12): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees,
Konnikova V.K. (SAI MSU).
Responsible Erkenov A.K.

(13-30): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(13-30): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Mikhailov A.G.

(01-15): Repairs,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-15): Adjustment, antenna measurements,
AMG, RAL (SAO RAS).
Responsible Zharov V.I., Trushkin S.

Feed-cabin 3

(01-30): The Sun five-azimuth observations 3.
Responsible Kazanina T.N.

(16-20): Reserve time (SAO RAS)

Feed-cabin 2

(21-30): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China)

(21-30): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Mikhailov A.G.

(21-30): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-15): Technical support,
MS R-600 (SAO RAS).
Responsible Yakovenko S.V., Shtondin A.F.

(01-15): Adjustment, antenna measurements,
AMG, RAL (SAO RAS).
Responsible Zharov V.I., Trushkin S.

(16-20): Reserve time

Feed-cabin 2

(21-30): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 5

(01-30): Test observations (SAO RAS).
Responsible Trushkin S.A.

D
E
C
E
M
B
E
R

Feed-cabin 1

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-20): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-20): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Mikhailov A.G.

(21-31): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees,
Konnikova V.K. (SAI MSU).
Responsible Erkenov A.K.

Feed-cabin 2

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-31): Radio properties of the blazars on the long time scales,
Mufakharov T..
Responsible Erkenov A.K.

(01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (SAO RAS; Metsahovi Radio Observatory, Finland).
Responsible Mikhailov A.G.

Feed-cabin 3

(01-31): The Sun multi-azimuth observations 3. Testing of the antenna system (South+Flat) in the tracking mode.
Responsible Kazanina T.N.

Feed-cabin 2

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 5

(01-31): Test observations (SAO RAS).
Responsible Trushkin S.A.

1 - During a trigger.
2 - ICRANet Italy; University of Oxford UK; INAF-IAPS Italy; SAO USA; Finnish Center for Astronomy with ESO FINCA.
3 - Structure and evolution of solar active regions (Alissandrakis C., University of Ioannina, Greece); Magnetosphere of the active region in a wide frequency range (Bogod V.M., SAO RAS); Study of the solar floccules in the CaIIK line and in the microwave range with GAS GAO and RATAN-600 (Tlatov A.G., GAO RAS); Investigation of ultra-weak solar activity (Lesovoy S.V., ISTP SB RAS); Study of the chromosphere and the transition region of sunspots with ALMA interferometer and RATAN-600 (M. Lukicheva, NJIT, USA).
4 - NRAO, USA; Shanghai Astronomical Observatory, China; Max-Planck-Insitut für Radioastronomie, Germany; Joint Institute for VLBI in Europe; IRA INAF, Italy; Netherlands Institute for Radio Astronomy, Netherlands.

Feed-cabin 1 - secondary mirror with complex equipment of the continuous spectrum of 1.28-21.7 GHz.
Feed-cabin 2 - secondary mirror with complex equipment of the continuous spectrum of 2.25-21.7 GHz (ERIDAN).
Feed-cabin 3 - secondary mirror with solar spectral-polarization complex.